Image de couverture de livre

Exploring Milky Way rotation curves with Gaia DR3: a comparison between $Λ$CDM, MOND, and General Relativistic approaches

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Beordo, William, Crosta, Mariateresa, Lattanzi, Mario Gilberto
Format:	Preprint
Publié:	2024
Sujets:	Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
par: Beordo, William, et autres
Publié: (2025)

Cosmological implications of the Gaia Milky Way declining rotation curve
par: Coquery, Even, et autres
Publié: (2024)

Analysis of the plane of satellites around Milky Way-like galaxies in $Λ$CDM cosmology
par: Zhao, Xinghai, et autres
Publié: (2025)

Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison
par: Singh, Aryan, et autres
Publié: (2026)

Wide Binaries from Gaia DR3 : testing GR vs MOND with realistic triple modelling
par: Pittordis, Charalambos, et autres
Publié: (2025)

A MOND model applied to the rotation curve of galaxies
par: Ciqueira, Ana C. M., et autres
Publié: (2025)

A Relativistic MOND
par: Singh, Tejinder P.
Publié: (2026)

A comparison of pre-existing $Λ$CDM predictions with the abundance of {\it JWST} galaxies at high redshift
par: Lu, Shengdong, et autres
Publié: (2024)

Galaxy rotation curve in hyperconical universes: a natural relativistic MOND
par: Monjo, Robert
Publié: (2024)

Dynamical History of the Local Group in $Λ$CDM
par: Banik, Indranil, et autres
Publié: (2015)

Forward-modelling Milky Way Cepheids: selection effects and physical priors in the Gaia-HST calibration
par: Stiskalek, Richard, et autres
Publié: (2026)

Testing a proposed "planarity" tool for studying satellite systems: On the alleged consistency of Milky Way satellite galaxy planes with $Λ$CDM
par: Pawlowski, Marcel S., et autres
Publié: (2024)

The odd primordial halo of the Milky Way implied by Gaia. A shallow core, but a steep decline
par: Li, Pengfei, et autres
Publié: (2025)

Milky Way-est: Cosmological Zoom-in Simulations with Large Magellanic Cloud and Gaia-Sausage-Enceladus Analogs
par: Buch, Deveshi, et autres
Publié: (2024)

The Filament Rift: $Λ$CDM's Structural Challenge Against Observation
par: Tavasoli, Saeed, et autres
Publié: (2025)

That's so Retro: The Gaia-Sausage-Enceladus Merger Trajectory as the Origin of the Chemical Abundance Bimodality in the Milky Way Disk
par: Johnson, James W., et autres
Publié: (2025)

An analytic surface density profile for $Λ$CDM halos and gravitational lensing studies
par: Lazar, Alexandres, et autres
Publié: (2023)

Weighing Milky Way and Andromeda in an expanding $Λ$CDM Universe: Decreasing the Local Group mass
par: Benisty, David
Publié: (2024)

Exploring the fate of primordial discs in Milky Way-sized galaxies with the GigaEris simulation
par: van Donkelaar, Floor, et autres
Publié: (2024)

The Milky Way is a less massive galaxy--new estimates of the Milky Way's local and global stellar masses
par: Lian, Jianhui, et autres
Publié: (2025)

Microlensing of dark matter models in the Milky Way
par: Li, Bichu, et autres
Publié: (2025)

GD-1 and the Milky Way Starless Subhalos
par: Carlberg, Raymond G.
Publié: (2025)

EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
par: Wang, Yunchong, et autres
Publié: (2024)

How Early Could the Milky Way's Disk Form?
par: Semenov, Vadim A., et autres
Publié: (2024)

Dark matter distribution in Milky Way-analog galaxies
par: de Isídio, Natanael G., et autres
Publié: (2023)

Cosmoglobe DR2. IV. Modelling starlight in DIRBE with Gaia and WISE
par: Galloway, M., et autres
Publié: (2026)

Variable gravitational potential of Milky Way analogues in HESTIA suite
par: Arakelyan, Naira R., et autres
Publié: (2024)

Probing the magneto-ionic medium of the Milky Way using pulsars
par: Dhakal, Saakshi, et autres
Publié: (2025)

Matching JWST UV Luminosity Functions with Refined $Λ$CDM Halo Models
par: Fakhry, Saeed, et autres
Publié: (2025)

Classifying globular clusters and applying them to estimate the mass of the Milky Way
par: Sun, GuangChen, et autres
Publié: (2022)

The effect of environment on the mass assembly history of the Milky Way and M31
par: Wempe, Ewoud, et autres
Publié: (2025)

Finding accreted stars in the Milky Way: clues from NIHAO simulations
par: Buder, Sven, et autres
Publié: (2024)

Signatures of Galactic Expansion in Gaia DR3: Implications for the JWST Early-Galaxy Puzzle
par: Karapetian, G. S., et autres
Publié: (2025)

A consistent MOND modelling of the Bullet Cluster
par: Hernandez, X.
Publié: (2026)

Gravitational imaging through a triple source plane lens: revisiting the $Λ$CDM-defying dark subhalo in SDSSJ0946+1006
par: Ballard, Daniel J., et autres
Publié: (2023)

Model independent approach for calculating galaxy rotation curves for low $S/N$ MaNGA galaxies
par: Park, Sangwoo, et autres
Publié: (2024)

The Baryonic Mass Estimates of the Milky Way Halo in the form of High Velocity Clouds
par: Tahir, Noraiz, et autres
Publié: (2024)

The oldest Milky Way stars: New constraints on the age of the Universe and the Hubble constant
par: Tomasetti, Elena, et autres
Publié: (2025)

In-situ globular clusters in alternative dark matter Milky Way galaxies: a first approach to fuzzy and core-like dark matter theories
par: Boldrini, Pierre, et autres
Publié: (2025)

SPARC galaxies prefer Dark Matter over MOND
par: Khelashvili, Mariia, et autres
Publié: (2024)